K. Dolag

3.7k total citations
40 papers, 1.6k citations indexed

About

K. Dolag is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, K. Dolag has authored 40 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 36 papers in Astronomy and Astrophysics, 16 papers in Nuclear and High Energy Physics and 11 papers in Instrumentation. Recurrent topics in K. Dolag's work include Galaxies: Formation, Evolution, Phenomena (32 papers), Cosmology and Gravitation Theories (14 papers) and Astrophysics and Cosmic Phenomena (14 papers). K. Dolag is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (32 papers), Cosmology and Gravitation Theories (14 papers) and Astrophysics and Cosmic Phenomena (14 papers). K. Dolag collaborates with scholars based in Germany, Italy and United States. K. Dolag's co-authors include L. Moscardini, M. Kachelrieß, G. Brunetti, R. Cassano, Roberto Tomás, S. Ostapchenko, F. Govoni, L. Feretti, Gianluca Setti and P. Mazzotta and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

K. Dolag

38 papers receiving 1.5k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
K. Dolag Germany 22 1.5k 738 281 64 38 40 1.6k
M. De Petris Italy 19 937 0.6× 256 0.3× 306 1.1× 69 1.1× 37 1.0× 97 1.0k
Harry Desmond United Kingdom 18 926 0.6× 416 0.6× 219 0.8× 63 1.0× 54 1.4× 54 1.0k
Hubert Lampeitl United States 12 1.9k 1.3× 851 1.2× 344 1.2× 44 0.7× 47 1.2× 13 1.9k
M. Rossetti Italy 23 1.4k 1.0× 552 0.7× 377 1.3× 61 1.0× 30 0.8× 63 1.5k
Jean‐Michel Alimi France 19 987 0.7× 524 0.7× 162 0.6× 141 2.2× 27 0.7× 115 1.1k
Emanuele Castorina Italy 19 913 0.6× 508 0.7× 186 0.7× 71 1.1× 28 0.7× 39 1.0k
Veronica Biffi Italy 22 1.2k 0.9× 270 0.4× 506 1.8× 69 1.1× 25 0.7× 49 1.3k
A. Kashlinsky United States 22 1.5k 1.0× 726 1.0× 205 0.7× 69 1.1× 32 0.8× 63 1.6k
M. Dessauges‐Zavadsky Switzerland 29 2.3k 1.6× 364 0.5× 598 2.1× 32 0.5× 80 2.1× 89 2.4k
Alexander M. Beck Germany 16 1.0k 0.7× 279 0.4× 364 1.3× 55 0.9× 19 0.5× 21 1.1k

Countries citing papers authored by K. Dolag

Since Specialization
Citations

This map shows the geographic impact of K. Dolag's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by K. Dolag with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites K. Dolag more than expected).

Fields of papers citing papers by K. Dolag

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by K. Dolag. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by K. Dolag. The network helps show where K. Dolag may publish in the future.

Co-authorship network of co-authors of K. Dolag

This figure shows the co-authorship network connecting the top 25 collaborators of K. Dolag. A scholar is included among the top collaborators of K. Dolag based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with K. Dolag. K. Dolag is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Dolag, K., Matías Bravo, A. S. G. Robotham, et al.. (2025). Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys. Astronomy and Astrophysics. 694. A207–A207. 4 indexed citations
2.
Dolag, K., et al.. (2025). Simulating the LOcal Web (SLOW). Astronomy and Astrophysics. 702. A243–A243.
3.
Dolag, K., et al.. (2025). The impact of assembly history on the X-ray detectability of halos. Astronomy and Astrophysics. 698. A191–A191. 1 indexed citations
4.
Dolag, K., et al.. (2025). Radial X-ray profiles of simulated galaxies. Astronomy and Astrophysics. 695. A2–A2. 5 indexed citations
5.
Gozaliasl, G., A. Finoguenov, O. Ilbert, et al.. (2024). COSMOS brightest group galaxies. Astronomy and Astrophysics. 690. A315–A315. 1 indexed citations
6.
Brown, Shea, Tessa Vernstrom, E. Carretti, et al.. (2017). Limiting magnetic fields in the cosmic web with diffuse radio emission. Monthly Notices of the Royal Astronomical Society. 468(4). 4246–4253. 45 indexed citations
7.
Meneghetti, M., Elena Rasia, Julian Merten, et al.. (2010). Weighing simulated galaxy clusters using lensing and X-ray. Astronomy and Astrophysics. 514. A93–A93. 171 indexed citations
8.
Govoni, F., K. Dolag, M. Murgia, et al.. (2010). Rotation measures of radio sources in hot galaxy clusters. Astronomy and Astrophysics. 522. A105–A105. 52 indexed citations
9.
Brunetti, G., R. Cassano, K. Dolag, & Gianluca Setti. (2009). On the evolution of giant radio halos and their connection with cluster mergers. Astronomy and Astrophysics. 507(2). 661–669. 110 indexed citations
10.
Maio, Umberto, B. Ciardi, K. Dolag, & L. Tornatore. (2008). Cooling in Primordial Structure Formation. AIP conference proceedings. 33–35. 2 indexed citations
11.
Gitti, Myriam, et al.. (2008). The complex galaxy cluster Abell 514: New results obtained with the XMM-Newton satellite. Astronomy and Astrophysics. 490(2). 537–545. 3 indexed citations
12.
Branchini, E., et al.. (2008). The mass density field in simulated non-Gaussian scenarios. Monthly Notices of the Royal Astronomical Society. 390(1). 438–446. 29 indexed citations
13.
Maturi, M., L. Moscardini, P. Mazzotta, K. Dolag, & G. Tormen. (2007). The importance of merging activity for the kinetic polarization of the Sunyaev-Zel'dovich signal from galaxy clusters. Astronomy and Astrophysics. 475(1). 71–81. 5 indexed citations
14.
Govoni, F., M. Murgia, L. Feretti, et al.. (2006). The intracluster magnetic field power spectrum in Abell 2255. Astronomy and Astrophysics. 460(2). 425–438. 98 indexed citations
15.
Maturi, M., M. Meneghetti, Matthias Bartelmann, K. Dolag, & L. Moscardini. (2005). An optimal filter for the detection of galaxy clusters through weak lensing. Springer Link (Chiba Institute of Technology). 42 indexed citations
16.
Dolag, K., F. K. Hansen, M. Roncarelli, & L. Moscardini. (2005). The imprints of local superclusters on the Sunyaev-Zel'dovich signals and their detectability with Planck. Monthly Notices of the Royal Astronomical Society. 363(1). 29–39. 57 indexed citations
17.
Reinecke, M., K. Dolag, R. Hell, Matthias Bartelmann, & T. A. Enßlin. (2005). A simulation pipeline for the Planck mission. Astronomy and Astrophysics. 445(1). 373–373. 29 indexed citations
18.
Meneghetti, M., Matthias Bartelmann, K. Dolag, et al.. (2005). Strong lensing efficiency of galaxy clusters in dark energy cosmologies. Astronomy and Astrophysics. 442(2). 413–422. 30 indexed citations
19.
Dolag, K., et al.. (2005). Simulating the magnetic field in the local supercluster. Max Planck Institute for Plasma Physics. 1–6. 2 indexed citations
20.
Dolag, K., S. Schindler, F. Govoni, & L. Feretti. (2001). Correlation of the magnetic field and the intra-cluster gas density ingalaxy clusters. Springer Link (Chiba Institute of Technology). 76 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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